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A Grid of NLTE Line-Blanketed Model Atmospheres of Early B-type Stars
Thierry Lanz, Ivan Hubeny
We have constructed a comprehensive grid of 1540 metal line-blanketed, NLTE, plane-parallel, hydrostatic model atmospheres for the basic parameters appropriate to early B-type star…
Theory for the Secondary Eclipse Fluxes, Spectra, Atmospheres, and Light Curves of Transiting Extrasolar Giant Planets
A. Burrows, D. Sudarsky, I. Hubeny
We have created a general methodology for calculating the wavelength-dependent light curves of close-in extrasolar giant planets (EGPs) as they traverse their orbits. Focussing on…
Neon Abundances in B-Stars of the Orion Association: Solving the Solar Model Problem?
Katia Cunha, Ivan Hubeny, Thierry Lanz
We report on non-LTE Ne abundances for a sample of B-type stellar members of the Orion Association. The abundances were derived by means of non-LTE fully metal-blanketed model atmo…
New Praesepe white dwarfs and the initial mass-final mass relation
P. D. Dobbie, R. Napiwotzki, M. R. Burleigh +6
We report the spectroscopic confirmation of four further white dwarf members of Praesepe. This brings the total number of confirmed white dwarf members to eleven making this the se…
A Grid of Relativistic, non-LTE Accretion Disk Models for Spectral Fitting of Black Hole Binaries
Shane W. Davis, Ivan Hubeny
Self-consistent vertical structure models together with non-LTE radiative transfer should produce spectra from accretion disks around black holes which differ from multitemperature…